Static black holes in two-dimensional string theory can carry tachyon
hair. Configurations which are nonsingular at the event horizon have a
nonvanishing asymptotic energy density. Such solutions can be smoothl
y extended through the event horizon and have a nonvanishing energy fl
ux emerging from the past singularity. Dynamical processes will not ch
ange the amount of tachyon hair on a black hole. In particular, there
will be no tachyon hair on a black hole formed in gravitational collap
se if the initial geometry is the linear dilaton vacuum. There also ex
ist static solutions with a finite total energy, which have singular e
vent horizons. Simple dynamical arguments suggest that black holes for
med in gravitational collapse will not have tachyon hair of this type.